r114_d6.0_Z

There is no treatment for a luminous central remnant included in the radiative transfer simulation of this model. The radiative transfer for this model was originally simulated for the Lach et al. (2022) pure deflagration parameter study. However, the radiative transfer was simulated again for this study so that it extends to later times. This allows the comparisons of this model and the new models presented in this study (which include treatment for a luminous central remnant in the radiative transfer) to be extended to later epochs.

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r114_d6.0_Z angle averaged light curves

  • Description: Light curve file format: Table with 15 columns. The first column gives the time since explosion in days, the second column gives the absolute bolometric magnitude and the remaining columns give the absolute magnitudes for the bands specified in the header line.
  • Date uploaded: April 9, 2024, 12:10 p.m.
    • r114_d6.0_Z angle averaged light curves
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    r114_d6.0_Z angle averaged optical spectral time-series

  • Description: Optical spectral time-series file format: Table with 1+n columns and 1+m lines specifying the optical spectral time series for n epochs on m wavelength bins. The first line defines the time of the n epochs for which spectra have been calculated (time in days since explosion, the first 0.00 is a dummy value). The following m lines contain the fluxes for the various time steps for a given wavelength bin. The first column gives the wavelength in A, followed by n columns giving the fluxes (in units of erg/cm^2/s/A assuming a distance of 10pc).
  • Date uploaded: April 9, 2024, 12:11 p.m.
    • r114_d6.0_Z angle averaged optical spectral time-series
    Interactive plot Download spectrum file